| Start Date | Context | Status | Description |
|---|---|---|---|
| 2025-12-01 | hst_1298.pmap | latest | Delivery of new STIS CCD bias and dark reference files for CCD data taken between October 31 and November 11, 2025. The files were generated from data taken in the same time frame under STIS calibration programs 17633 and 17631. |
| 2025-11-24 | hst_1297.pmap | archived | The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on November 17, 2025, and should be used to calibrate ACS WFC observations taken between October 22, 2025 and November 17, 2025. |
| 2025-11-21 | hst_1296.pmap | archived | These WFC3 UVIS superdarks will affect all UVIS data taken from October 16, 2025 to November 9, 2025. Currently, the automated calibration pipeline and CRDS have only WFC3 UVIS drk and dkc reference files with USEAFTER dates of up to October 13, 2025. The automated pipeline should now use these reference files to perform dark subtraction on any UVIS datasets obtained between the dates above, as they represent the most accurate picture of dark current and hot pixels for this time period. These WFC3 UVIS drk and dkc files were generated using dark exposures from HST Cycle 32 CAL program 17669. More information regarding the method used to create the UVIS dark calibration reference files can be found in WFC3 ISR 2016-08. Additionally, the header of each reference file contains a detailed history section outlining the process, and provides a list of data used to create each file. This new bad pixel table with USEAFTER of October 16, 2025 was generated using data taken from October 17, 2025, through November 11, 2025. Currently, the Calibration Reference Data System only has WFC3 UVIS bad pixel reference tables up to a USEAFTER date of September 19, 2025. The automated pipeline should now use this reference file as the bad pixel table on any UVIS datasets obtained from October 17, 2025 to present because it represents the most accurate measure of pixel stability at the time of the science observation. These WFC3 UVIS bad pixel files were generated using 900 second dark exposures from the HST Cycle 32 daily monitoring programs 17665 and 17669. More information about the UVIS bad pixel tables is outlined in the WFC3 ISR 2018.15 and WFC3 ISR 2021.14. |
| 2025-11-03 | hst_1294.pmap | archived | Delivery of new STIS CCD bias and dark reference files for CCD data taken between September 30, 2025 and October 31, 2025. The files were generated from data taken in the same time frame under STIS calibration programs 17631 and 17633. |